NTT service mode observations of the Lyman-limit absorber towards Q1205-30.

Details NTT service mode observations of the Lyman-limit absorber towards Q1205-30. NTT service mode observations of the Lyman-limit absorber towards Q1205-30.

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999msngr..95...32f&link_type=abstract

The Messenger, vol. 95, p. 32-33

Physics

2

Quasars: Lyman-Alpha Systems, Quasars: Absorption Lines, Quasars: Emission Lines, Quasars: Redshifts

Scientific paper

In order to examine whether zabs ≍ zem systems indeed are more active emitters (e.g. due to photoionisation by the QSO or induced star formation) the authors choose to study Q1205-30, since the spectrum of Q1205-30 published by Lanzetta et al. (1991) shows the presence of a strong LLS at the emission redshift of the QSO, which is zem = 3.036. In this paper the authors report on preliminary results of the analysis of the data obtained during NTT service observation in January, February and March 1998.

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